activity
20242026
collaborators

6 papers

astro-ph.SR2026

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars

C. Martínez-Sebastián, R. Gamen, O. G. Benvenuto +6

For decades, the origin of helium enrichment in O-type stars has remained an open question. In this study, we investigate the correlation between surface helium abundance and orbit…

astro-ph.SR2026

The IACOB project: XVI. Surface helium abundances in Galactic O-type stars: indications for identifying binary interaction products

S. Simón-Díaz, G. Holgado, C. Martínez-Sebastián +13

The presence of massive O-type stars with surfaces enriched by CNO-cycle products has been known since the early 1980s. For many years, internal rotational mixing was assumed to be…

astro-ph.SR2026

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars

C. Martínez-Sebastián, G. Holgado, S. Simón-Díaz +2

Context. Growing evidence is revealing the crucial role of binarity in massive star evolution. This affects evolution models and demands a refinement of the available observational…

astro-ph.SR2025

The lack of fast rotators in Cyg OB2. I. Insights from spectral reclassification of its B0 population

D. Galán-Diéguez, S. R. Berlanas, A. Herrero +4

Context. Cygnus OB2, in the Cygnus X complex -- one of the most active star-forming regions of the Galaxy -- hosts hundreds of O- and B-type stars at different evolutionary stages.…

astro-ph.SR2025

An observational study of rotation and binarity of Galactic O-type runaway stars

M. Carretero-Castrillo, M. Ribó, J. M. Paredes +3

Gaia DR3 data have revealed new massive runaway stars, while spectroscopic surveys enable detailed characterization. The relative contributions of binary supernova (BSS) and dynami…

astro-ph.SR2024

The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction

C. Martínez-Sebastián, S. Simón-Díaz, H. Jin +4

There is increasing evidence that single-star evolutionary models are inadequate to reproduce all observational properties of massive stars. Binary interaction has emerged as a key…